{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:VU4JP34LLBD7AHANYLWTGXBL4Q","short_pith_number":"pith:VU4JP34L","schema_version":"1.0","canonical_sha256":"ad3897ef8b5847f01c0dc2ed335c2be429f2b9391bb68af01ac45fc4cfe59024","source":{"kind":"arxiv","id":"2001.06904","version":5},"attestation_state":"computed","paper":{"title":"UV & U-band luminosity functions from CLAUDS and HSC-SSP -- I. Using four million galaxies to simultaneously constrain the very faint and bright regimes to $z \\sim 3$","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Anneya Golob, Jean Coupon, Marcin Sawicki, Olivier Ilbert, St\\'ephane Arnouts, Stephen Gwyn, Thibaud Moutard, Xiaohu Yang","submitted_at":"2020-01-19T21:06:19Z","abstract_excerpt":"We constrain the rest-frame FUV (1546\\AA), NUV (2345\\AA) and U-band (3690\\AA) luminosity functions (LFs) and luminosity densities (LDs) with unprecedented precision from $z\\sim0.2$ to $z\\sim3$ (FUV, NUV) and $z\\sim2$ (U-band). Our sample of over 4.3 million galaxies, selected from the CFHT Large Area $U$-band Deep Survey (CLAUDS) and HyperSuprime-Cam Subaru Strategic Program (HSC-SSP) data lets us probe the very faint regime (down to $M_\\mathrm{FUV},M_\\mathrm{NUV},M_\\mathrm{U} \\simeq -15$ at low redshift) while simultaneously detecting very rare galaxies at the bright end down to comoving dens"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"2001.06904","kind":"arxiv","version":5},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2020-01-19T21:06:19Z","cross_cats_sorted":[],"title_canon_sha256":"d2c87a8d336625dd2be8279b9b70c88b42cc08682287edfbfae76764d840fd4d","abstract_canon_sha256":"4d6c6f1c98a5e3517ae973ba9109a97db745f8671fa0bb0cee4b1270bf8e6484"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:58:47.188242Z","signature_b64":"5vQ0C1oJB4iLLJvFooaWRoJcQ51PbRCUy9d+s6ogCxeitjSpIs3oI3K1+Jo9gbV1jN/xpvPvXFVy2mZMulx0AA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ad3897ef8b5847f01c0dc2ed335c2be429f2b9391bb68af01ac45fc4cfe59024","last_reissued_at":"2026-07-05T00:58:47.187798Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:58:47.187798Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"UV & U-band luminosity functions from CLAUDS and HSC-SSP -- I. Using four million galaxies to simultaneously constrain the very faint and bright regimes to $z \\sim 3$","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Anneya Golob, Jean Coupon, Marcin Sawicki, Olivier Ilbert, St\\'ephane Arnouts, Stephen Gwyn, Thibaud Moutard, Xiaohu Yang","submitted_at":"2020-01-19T21:06:19Z","abstract_excerpt":"We constrain the rest-frame FUV (1546\\AA), NUV (2345\\AA) and U-band (3690\\AA) luminosity functions (LFs) and luminosity densities (LDs) with unprecedented precision from $z\\sim0.2$ to $z\\sim3$ (FUV, NUV) and $z\\sim2$ (U-band). Our sample of over 4.3 million galaxies, selected from the CFHT Large Area $U$-band Deep Survey (CLAUDS) and HyperSuprime-Cam Subaru Strategic Program (HSC-SSP) data lets us probe the very faint regime (down to $M_\\mathrm{FUV},M_\\mathrm{NUV},M_\\mathrm{U} \\simeq -15$ at low redshift) while simultaneously detecting very rare galaxies at the bright end down to comoving dens"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2001.06904","kind":"arxiv","version":5},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2001.06904/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"2001.06904","created_at":"2026-07-05T00:58:47.187855+00:00"},{"alias_kind":"arxiv_version","alias_value":"2001.06904v5","created_at":"2026-07-05T00:58:47.187855+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2001.06904","created_at":"2026-07-05T00:58:47.187855+00:00"},{"alias_kind":"pith_short_12","alias_value":"VU4JP34LLBD7","created_at":"2026-07-05T00:58:47.187855+00:00"},{"alias_kind":"pith_short_16","alias_value":"VU4JP34LLBD7AHAN","created_at":"2026-07-05T00:58:47.187855+00:00"},{"alias_kind":"pith_short_8","alias_value":"VU4JP34L","created_at":"2026-07-05T00:58:47.187855+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/VU4JP34LLBD7AHANYLWTGXBL4Q","json":"https://pith.science/pith/VU4JP34LLBD7AHANYLWTGXBL4Q.json","graph_json":"https://pith.science/api/pith-number/VU4JP34LLBD7AHANYLWTGXBL4Q/graph.json","events_json":"https://pith.science/api/pith-number/VU4JP34LLBD7AHANYLWTGXBL4Q/events.json","paper":"https://pith.science/paper/VU4JP34L"},"agent_actions":{"view_html":"https://pith.science/pith/VU4JP34LLBD7AHANYLWTGXBL4Q","download_json":"https://pith.science/pith/VU4JP34LLBD7AHANYLWTGXBL4Q.json","view_paper":"https://pith.science/paper/VU4JP34L","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2001.06904&json=true","fetch_graph":"https://pith.science/api/pith-number/VU4JP34LLBD7AHANYLWTGXBL4Q/graph.json","fetch_events":"https://pith.science/api/pith-number/VU4JP34LLBD7AHANYLWTGXBL4Q/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VU4JP34LLBD7AHANYLWTGXBL4Q/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VU4JP34LLBD7AHANYLWTGXBL4Q/action/storage_attestation","attest_author":"https://pith.science/pith/VU4JP34LLBD7AHANYLWTGXBL4Q/action/author_attestation","sign_citation":"https://pith.science/pith/VU4JP34LLBD7AHANYLWTGXBL4Q/action/citation_signature","submit_replication":"https://pith.science/pith/VU4JP34LLBD7AHANYLWTGXBL4Q/action/replication_record"}},"created_at":"2026-07-05T00:58:47.187855+00:00","updated_at":"2026-07-05T00:58:47.187855+00:00"}